Fig. 15
Cumulative photon arrival time distributions as used for the KS tests. Source counts are plotted in black, the background light curve is shown in green. The distribution, expected from a constant source is shown in blue and the reference distribution in red. In case of a constant source and background light curve, all lines are blended. The source-count distribution of variable sources is significantly different from the expected distribution. Upper left: the bright foreground star N°2041. Lower left: the foreground star candidate N°255. Upper right: the HMXB RX J0054.9-7245 (N°335). Lower right: the SNR 1E0102.2-7219.
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